Atomic data for astrophysics : Ni XI.
Del Zanna, G. and Storey, P. J. and Badnell, Nigel (2014) Atomic data for astrophysics : Ni XI. Astronomy and Astrophysics, 566. A123. ISSN 0004-6361 (https://doi.org/10.1051/0004-6361/201423823)
Preview |
PDF.
Filename: DelZanna_etal_AA2014_atomic_data_astrophysics_Ni_XI.pdf
Final Published Version Download (308kB)| Preview |
Abstract
We present a new large-scale R-matrix scattering calculation for electron collisional excitation of Ni xi, carried out with the intermediate-coupling frame transformation method. The target includes all the main configurations up to n = 4, and is a significant improvement over earlier R-matrix (only three n = 3 configurations) and distorted-wave (DW) calculations. We find significant enhancements in the collision strengths of many of the strong transitions to the n = 3,4 levels. They are due to the resonances that arise within the present large-scale target. This results in significant increases in the predicted intensities of the UV and visible forbidden lines within the 3s23p53d configuration, the strong EUV lines that result from the decays of the 3s23p53d levels to the ground state, and the decays from the n = 4 levels, which are visible in the soft X-rays. We find good agreement between predicted and observed line intensities in the EUV. With the present atomic data, lines from Ni xi can reliably be used for plasma diagnostics. We also revise some level energies and suggest a few new possible identifications.
ORCID iDs
Del Zanna, G., Storey, P. J. and Badnell, Nigel ORCID: https://orcid.org/0000-0001-7418-7996;-
-
Item type: Article ID code: 51979 Dates: DateEvent23 June 2014Published30 April 2014AcceptedSubjects: Science > Astronomy
Science > PhysicsDepartment: Faculty of Science > Physics Depositing user: Pure Administrator Date deposited: 27 Feb 2015 12:08 Last modified: 15 Dec 2024 01:20 Related URLs: URI: https://strathprints.strath.ac.uk/id/eprint/51979